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The Be Phenomenon in A-type Supergiants

Published online by Cambridge University Press:  12 April 2016

Eva Verdugo ,
Antonio Talavera  and
Ana I. Gómez de Castro
Eva Verdugo
Affiliation:
ISO Data Centre, VILSPA, P.O. Box 50727, 28080 Madrid.Spain
Antonio Talavera
Affiliation:
LAEFF/INTA, VILSPA, P.O. Box 50727, 28080 Madrid.Spain
Ana I. Gómez de Castro
Affiliation:
Institute de Astronomía y Geodesia (CSIC-UCM), Fac. cc. Matemáticas, Universidad Complutense, Av. Complutense s/n, E-28040-Madrid.Spain

Abstract

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Multiwavelength observations of a large sample of A-type supergiants reveal that these stars display several features associated with the classical Be phenomenon.

Type
1. Overview
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 91 - 95
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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